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Cited by 374

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Gravitational waveforms from inspiralling compact binaries to second-post-Newtonian order

Open access
Blanchet, Luc, Iyer, Bala R, Will, Clifford M, Wiseman, Alan G·1996·Classical and Quantum Gravity
DOI 10.1088/0264-9381/13/4/002
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Abstract

The two independent `plus' and `cross' polarization waveforms associated with the gravitational waves emitted by inspiralling, non-spinning, compact binaries are presented, ready for use in the data analysis of signals received by future laser interferometer gravitational-wave detectors such as LIGO and VIRGO. The computation is based on a recently derived expression of the gravitational field at the second-post-Newtonian approximation of general relativity beyond the dominant (Newtonian) quadrupolar field. The use of these theoretical waveforms to make measurements of astrophysical parameters and to test the nature of relativistic gravity is discussed.

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Metadata

Authors
Blanchet, L., Iyer, B. R., Will, C. M., & Wiseman, A. G.
Venue
Classical and Quantum Gravity
Publisher
IOP Publishing
Published
1996-04-01
Volume
13
Issue
4
Pages
575-584
ISSN
  • 0264-9381 (ISSN-L)
  • 1361-6382
DOI
10.1088/0264-9381/13/4/002
OpenAlex
W2102464939
Cited by
374
References
0
FWCI
11.97
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Gravitational waveforms from inspiralling compact binaries to second-post-Newtonian order. https://app.cochat.ai/papers/10.1088/0264-9381/13/4/002
The paper
Blanchet, L., Iyer, B. R., Will, C. M., & Wiseman, A. G. (1996). Gravitational waveforms from inspiralling compact binaries to second-post-Newtonian order. Classical and Quantum Gravity. https://doi.org/10.1088/0264-9381/13/4/002

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.